Open Access

Table A.1

Orbital and physical parameters of the 64 transiting Kepler and K2 planets.

Name Tc Ρ Rp i Ref. e Κ Mp ρp log gp a Τeq Fp
[BJDTDB – 2.45E06] [day] [R] [deg] transits [m s−1] [M] [g cm−3] [cgs] [AU] [K] [F]
Kepler-10b 5034.08687(18) 0.83749070(20) 1 0 (fixed) 2.34 ±0.21 3.26 ± 0.30 0.01685 ± 0.00013 2188 ±16 3820 ± 120
Kepler-10c 5062.26648(81) 45.294301(48) 2.355 ± 0.022 89.623 ±0.011 1, 2 0.130 ±0.050 2.19 ±0.24 11.4 ± 1.3 0.2410 ±0.0019 578 ±4 18.68 ±0.57
Kepler-19b 4959.7074(14) 9.2869900(00) 2.209 ± 0.048 3, 4 < 0.41 3.1 ± 1.4 0.0846 ± 0.0012 851 ± 14 87.6 ± 6.0
Kepler-20b 4967.50225(33) 3.6961049(16) 5, 6 < 0.083 4.23 ± 0.54 9.7 ± 1.3 0.04565 ± 0.00089 1187 ±16 331 ± 19
Kepler-20c 4971.60886(16) 10.8540774(21) 5, 6 < 0.076 3.38 ±0.61 11.1 ±2.1 0.0936 ±0.0018 828 ±11 78.7 ± 4.6
Kepler-20d 4997.7296(11) 77.611455(96) 5, 6 < 0.082 2.12 ±0.57 0.3474 ± 0.0067 430 ±6 5.71 ± 0.33
Kepler-20e 4968.93956(34) 6.0984882(99) 0.821 ±0.022 5, 6 < 0.092 < 0.28 <0.76 < 7.5 < 3.0 0.0637 ± 0.0012 1004 ±14 169.8 ±9.8
Kepler-20f 4968.19883(57) 19.578328(48) 5, 6 < 0.094 < 0.35 < 1.4 < 8.4 < 3.2 0.1387 ± 0.0027 681 ±9 35.9 ±2.1
Kepler-21b 5093.83716(85) 2.7858212(32) 7 0 (fixed) 2.70 ± 0.46 7.5 ± 1.3 9.3 ± 1.6 2015 ±16 2749 ± 90
Kepler-22b 4966.7001(68) 289.863876(13) 2.10 ±0.12 8, 9, t.w.1 < 0.72 < 1.6 <9.1 < 5.2 < 3.3 279 ±4 1.013 ±0.060
Kepler-37b 5017.0473(37) 13.367020(60) 6, 10, t.w.1 < 0.098 < 0.25 <0.79 < 140 < 3.9 0.1019 ±0.0014 718 ± 10 44.5 ± 2.8
Kepler-37c 5024.83997(87) 21.301848(18) 6, 10, t.w.1 < 0.099 < 0.34 < 1.3 < 15 < 3.3 0.1390 ± 0.0020 615 ±9 23.9 ± 1.5
Kepler-37d 5008.24982(13) 39.7922622(65) 6, 10, t.w.1 < 0.10 < 0.44 <2.0 < 1.3 < 2.7 0.2109 ± 0.0030 499 ±7 10.39 ±0.65
Kepler-68b 5006.858780(76) 5.39875259(52) 2.357 ± 0.023 6, 11 < 0.090 2.83 ± 0.23 8.03 ± 0.67 0.06135 ± 0.00043 1275 ±17 441 ± 25
Kepler-68c 4969.3821(11) 9.605027(13) 0.979 ±0.019 6, 11 < 0.099 < 0.37 < 1.3 < 7.5 < 3.1 0.09008 ± 0.00063 1052 ±14 204 ± 12
Kepler-78b 4953.95984(15) 0.355007450(80) 1.201 ±0.028 12, t.w.1 0 (fixed) 1.75 ±0.28 1.68 ±0.27 2223 ± 32 4070 ± 240
Kepler-93b 4944.29227(13) 4.72673978(97) 1.478 ±0.019 89.183 ±0.044 13 0 (fixed) 1.89 ±0.21 4.66 ± 0.53 0.05343 ± 0.00065 1133 ±17 275 ± 18
Kepler-102b 4968.8696(11) 5.286965(12) 0.460 ± 0.026 89.78 ± 0.22 6, 14, t.w.1 < 0.100 < 0.47 < 1.1 <62 < 3.7 0.05521 ± 0.00049 857 ± 20 90.0 ± 9.0
Kepler-102c 4972.9746(24) 7.071392(22) 0.567 ± 0.028 89.82 ±0.15 6, 14, t.w.1 < 0.094 < 0.66 < 1.7 <52 < 3.7 0.06702 ± 0.00059 777 ± 18 61.0 ±6.1
Kepler-102d 4967.091280(00) 10.3117670(41) 1.154 ±0.058 89.49 ±0.11 6, 14, t.w.1 < 0.092 1.02 ±0.44 3.0 ± 1.3 0.08618 ± 0.00076 686 ± 16 36.9 ± 3.7
Kepler-102e 4967.75370(12) 16.1456994(22) 2.17 ±0.11 89.488 ± 0.051 6, 14, t.w.1 < 0.089 1.37 ±0.53 4.7 ± 1.8 0.1162 ±0.0010 590 ± 14 20.3 ± 2.0
Kepler- 102f 4978.0276(16) 27.453592(60) 0.861 ±0.022 89.320 ± 0.037 6, 14, t.w.1 < 0.10 < 1.1 <4.3 < 37 < 3.8 0.1656 ±0.0015 495 ± 11 10.0 ± 1.0
Kepler-103b 5677.65243(28) 15.9653287(92) 15 < 0.093 2.21 ±0.88 9.8 ±3.9 973 ± 13 149.9 ± 8.6
Kepler-103c 5667.15973(44) 179.60978(20) 5.45 ±0.18 15 < 0.095 3.8 ± 1.7 434.0 ± 6.0 5.95 ± 0.34
Kepler-107b 5701.08414(37) 3.1800218(29) 1.536 ±0.025 89.05 ± 0.67 16 < 0.10 1.44 ±0.68 0.04544 ± 0.00036 1592 ± 19 1073 ±53
Kepler-107c 5697.01829(79) 4.9014520(00) 1.597 ±0.026 16 < 0.080 3.29 ± 0.66 10.0 ±2.0 0.06064 ± 0.00048 1378 ± 16 602 ± 30
Kepler-107d 5702.9547(60) 7.95839(12) 0.860 ± 0.060 16 < 0.11 < 2.1 <7.7 < 67 < 4.0 0.08377 ± 0.00065 1173 ± 14 315 ± 16
Kepler-107e 5694.48550(46) 14.749143(19) 2.903 ± 0.035 89.67 ± 0.22 16 < 0.10 3.22 ± 0.74 14.1 ±3.3 0.12638 ± 0.00099 955 ± 11 138.7 ±6.8
Kepler-109b 4955.97791(60) 6.4816307(48) 2.49 ±0.11 87.06 ±0.11 6, 14, t.w.1 < 0.11 < 1.6 <4.9 < 1.7 < 2.9 0.0701 ±0.0019 1276 ± 23 442 ± 34
Kepler-109c 4970.5722(10) 21.222650(27) 2.65 ±0.12 89.63 ±0.19 6, 14, t.w.1 < 0.098 < 1.8 < 8.2 < 2.4 < 3.1 0.1546 ± 0.0042 859 ± 16 91.0 ±7.1
Kepler-323b 4953.9478(14) 1.6783280(15) 1.381 ±0.035 9, 17, t.w.1 < 0.095 < 2.1 <3.9 < 8.2 < 3.3 0.02778 ± 0.00068 1838 ±35 1900 ± 150
Kepler-323c 4956.9823(20) 3.5538229(22) 1.570 ±0.040 88.7 ± 1.3 9, 17, t.w.1 < 0.095 2.8 ±1.4 0.0458 ±0.0011 1431 ± 27 700 ± 56
Kepler-409b 5012.0829(34) 68.9583216(39) 1.199 ±0.043 86.30 ±0.13 9, 14, t.w.1 < 0.69 < 1.6 <6.0 < 19 < 3.6 0.3192 ± 0.0060 438 ±7 6.15 ±0.42
Kepler-454b 5008.06758(77) 10.5737534(78) 2.37 ±0.13 87.90 ± 0.20 18 < 0.32 1.64 ±0.41 5.4 ± 1.4 916 ± 10 117.7 ±5.6
Kepler-538b 5044.6789(11) 81.73778(13) 19 < 0.21 2.09 ± 0.47 12.9 ±2.9 6.5 ±1.5 417 ±5 5.07 ± 0.29
Kepler-1655b 5013.89795(69) 11.8728787(85) 2.213 ±0.082 87.62 ± 0.55 20 < 0.19 1.51 ±0.48 5.4 ± 1.7 0.1029 ±0.0014 938 ± 15 129.1 ± 8.8
Kepler-1876b 4971.0510(50) 6.992050(38) 21, t.w.1 < 0.098 < 0.71 <2.4 < 19 < 3.5 0.0758 ±0.0019 1299 ± 22 475 ± 34
K2-2b/HIP 116454b 6907.887(29) 9.0949(26) 2 2.53 ±0.18 88.43 ± 0.40 22 < 0.089 3.73 ± 0.42 0.07765 ± 0.00093 745 ± 15 51.4 ±4.3
K2-3b 6813.41843(39) 10.0546260(00) 2.25 ± 0.23 23, t.w.1 < 0.094 2.66 ± 0.37 3.10 ±0.11 0.0778 ± 0.0026 513 ±29
K2-3c 6812.28013(95) 24.646582(39) 1.69 ±0.17 23, t.w.1 < 0.095 1.01 ±0.35 3.3 ± 1.2 0.1414 ± 0.0047 381 ±21
K2-3d 6826.22347(53) 44.556456(97) 1.62 ±0.18 23, t.w.1 < 0.097 <0.39 < 1.6 < 2.1 <2.8 0.2097 ± 0.0070 312 ±17
K2-12b 6815.3701(29) 8.28246(52) 24, t.w.1 <0.50 < 2.1 <5.2 < 1.6 <2.9 1026±15 185 ± 12
K2-36b 6810.8916(13) 1.422614(38) 1.430 ±0.080 25 < 0.093 2.85 ± 0.92 4.3 ± 1.4 0.02288 ± 0.00010 1328±12 519 ±20
K2-36c 6812.84001(71) 5.340888(86) 3.20 ± 0.30 25 < 0.089 3.4 ± 1.2 7.9 ±2.8 0.05528 ± 0.00023 854 ± 8 89.0 ± 3.4
K2-38b 6896.8786(54) 4.01593(50) 1.655 ±0.096 26, 27, t.w.1 < 0.11 3.02 ± 0.43 0.0503 ±0.0011 1310 ±22 490 ± 35
K2-38c 6900.4752(33) 10.56103(90) 2.49 ± 0.22 26, 27, t.w.1 < 0.086 2.11 ±0.37 3.07 ±0.11 0.0959 ± 0.0022 949 ± 16 135.3 ±9.5
K2-79b 7103.22750(84) 10.99470(47) 88.44 ± 0.44 28 < 0.23 2.63 ± 0.69 9.2 ±2.4 1022 ± 20 181 ± 15
K2-96b/HD 3167b 7394.37454(43) 0.959641(11) 29, t.w.1 0 (flxed) 3.56 ±0.15 1774 ±29 1650±110
K2-96c/HD 3167c 7394.9788(12) 29.8454(12) 29, t.w.1 < 0.060 2.58 ±0.15 564 ±9 16.9 ± 1.1
K2-106b 7394.01140(00) 0.571292(12) 1.725 ±0.039 30, t.w.1 0 (flxed) 6.50 ± 0.52 2300 ± 36 4670 ± 300
K2-106c 7405.7316(44) 13.33970(96) 30, t.w.1 < 0.13 2.48 ± 0.66 8.9 ±2.4 805 ±12 70.0 ± 4.5
K2-110b 7275.32992(61) 13.86375(26) 31 < 0.13 5.25 ± 0.89 15.9 ±2.7 0.10207 ± 0.00083 638 ±11 27.7 ± 2.0
K2-lllb 7100.0768(19) 5.35180(40) 32 < 0.100 2.30 ± 0.30 0.05650 ± 0.00045 1309±19 490 ± 30
K2-131b 7582.9360(11) 0.3693038(91) 33, t.w.1 0 (flxed) 8.0 ± 1.3 7.9 ± 1.3 0.00936 ± 0.00014 2223 ± 37 4070 ± 280
K2- 135b /GJ 9827b 7738.82586(26) 1.2089819(71) 34 < 0.063 4.31 ± 0.39 5.14 ±0.47 0.01880 ± 0.00016 1175±14 318 ± 16
K2-135c/GJ9827c 7742.19930(73) 3.648096(63) 34 < 0.094 <0.75 < 1.3 < 3.7 < 2.9 0.03925 ± 0.00033 813 ±10 73.0 ± 3.7
K2-135d/GJ9827d 7740.96115(45) 6.201470(63) 87.443 ± 0.045 34 < 0.13 1.73 ±0.43 0.05590 ± 0.00046 681 ± 8 36.0 ± 1.9
K2-141b 7744.07160(22) 0.2803244(15) 1.510 ±0.050 35 0 (flxed) 6.10 ±0.39 0.00747 ± 0.00010 2103 ±56
K2-141c 7751.15460(00) 7.74850(22) 35 < 0.092 < 3.2 < 8.0 < 0.081 < 1.9 0.06830 ± 0.00091 695 ±18 39.1 ±4.3
K2-167b 6979.9368(25) 9.97748(00) 24, t.w.1 < 0.47 0.0910 ± 0.0025 1174 ±24 317 ±27
K2-222b 7399.0595(16) 15.38857(88) 28 < 0.16 2.29 ± 0.43 8.7 ± 1.7 0.1206 ± 0.0029 871 ±23
K2-262b/Wolf503b 8191.36145(11) 6.001270(21) 2.043 ± 0.069 89.87 ±0.13 36 0.409 ± 0.085 3.11 ±0.39 789 ±16 64.7 ± 5.5
K2-263b 8111.1274(12) 50.818947(94) 2.41 ±0.12 37 < 0.15 2.83 ± 0.39 14.9 ±2.1 0.2573 ± 0.0030 470 ±7 8.17 ±0.52
K2-312b/HD 80653b 8134.42440(70) 0.719573(21) 1.613 ±0.071 82.1 ±2.4 38 0 (flxed) 3.62 ±0.21 0.01661 ± 0.00019 2463 ± 30 6130 ±310
K2-418b/EPIC-22…35b 7920.44584(80) 16.141132(19) 39 <0.23 2.76 ± 0.39 0.1237 ±0.0017 804 ± 10 69.7 ± 3.7

Notes. From left to right, the columns report the planet name, the transit mid-time, the orbital period, the planetary radius, the orbital inclination, the references for the transit parameters, the orbital eccentricity, the radial-velocity semi-amplitude, the planet mass, density and surface gravity, the semi-major axis, the equilibrium temperature by considering a null Bond albedo and full heat redistribution from the day to the night side, and the stellar incident flux. Table also available at the CDS.

1 This work: the planet radius was newly determined from the Rp/Rs transit parameter in the literature and the stellar radius Rs as reported in Table 1. 2The orbital period of K2-2b comes from the RVs by imposing a Gaussian prior on Tc only, and slightly differs from the value reported in Vanderburg et al. (2015), which is affected by systematics in the photometric data of the MOST satellite (A. Vanderburg, private communication).

References. (1) Dumusque et al. 2014; (2) Bonomo et al. (in prep.); (3) Ballard et al. 2011; (4) Malavolta et al. 2017; (5) Buchhave et al. 2016; (6) Gajdoš et al. 2019 (7) López-Morales et al. 2016; (8) Borucki et al. 2012; (9) Holczer et al. 2016; (10) Barclay et al. 2013; (11) Margini et al. (in prep.); (12) Howard et al. 2013; (13) Ballard et al. 2014; (14) Marcy et al. 2014; (15) Dubber et al. 2019; (16) Bonomo et al. 2019; (17) Rowe et al. 2015; (18) Gettel et al. 2016; (19) Mayo et al. 2019; (20) Haywood et al. 2018; (21) Coughlin et al. 2016; (22) Vanderburg et al. 2015; (23) Kosiarek et al. 2019; (24) Mayo et al. 2018; (25) Damasso et al. 2019; (26) Sinukoff et al. 2016; (27) Toledo-Padrón et al. 2020; (28) Nava et al. 2022; (29) Christiansen et al. 2017; (30) Guenther et al. 2017; (31) Osborn et al. 2017; (32) Mortier et al. 2020; (33) Dai et al. 2017; (34) Rice et al. 2019; (35) Malavolta et al. 2018; (36) Polanski et al. 2021; (37) Mortier et al. 2018; (38) Frustagli et al. 2020; (39) Tronsgaard et al. (in prep.);

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